The mass-metallicity relation at z ≁ 0.7

被引：0

作者：

Savaglio, S ^{[1
]}

Glazebrook, K ^{[1
]}

Le Borgne, D ^{[1
]}

Juneau, S ^{[1
]}

Abraham, RG ^{[1
]}

Crampton, D ^{[1
]}

McCarthy, PJP ^{[1
]}

Chen, HW ^{[1
]}

Marzke, R ^{[1
]}

Carlberg, RG ^{[1
]}

Jorgensen, I ^{[1
]}

Roth, K ^{[1
]}

Hook, I ^{[1
]}

Murowinski, R ^{[1
]}

机构：

[1] Johns Hopkins Univ, Baltimore, MD 21218 USA

来源：

SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: CONFRONTING MODELS WITH DATA | 2005年 / 761卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The ISM metallicity and the stellar mass are examined in a sample of 66 galaxies at 0.4 < z < 1, selected from the Gemini Deep Deep Survey (GDDS) and the Canada-France Redshift Survey (CFRS). We observe a mass-metallicity relation similar to that seen in z similar to 0.1 SDSS galaxies, but displaced towards higher masses and/or lower metallicities. Using this sample, and a small sample of z similar to 2.3 LBGs, a redshift dependent mass-metallicity relation is proposed which describes the observed results.

引用

页码：425 / 428

页数：4

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